The Giant Magellan Telescope. Status

The Giant Magellan Telescope. Status By Dr. Mauricio Pilleux Head of Administration (Chile) GMTO Corporation [email protected] April 17, 2019 Observatories in Chile: The beginnings … a successful experiment Cerro Tololo Interamerican Observatory AURA, 1962 Magellan telescopes, 2000 Las Campanas Carnegie Institution of Washington, 1968 La Silla ESO, 1969 2 Observatories in Chile: “Second stage” Very Large Telescope (VLT) Cerro Paranal, ESO, 1999 Gemini South Cerro Pachón, 2002 (AURA) ALMA NRAO-ESO-NAOJ, 2013 3 Observatories in Chile: “Stage 3.0” – big, big, big Giant Magellan Telescope (GMT) Cerro Las Campanas, 2023 (GMTO Corporation) European- Extremely Large Telescope (EELT) Cerro Armazones, 2026 (ESO) Large Synoptic Survey Telescope (LSST) Cerro Pachón, 2022 (NSF/AURA-DOE/SLAC) 4 What next? Size (physical) GMT TMT EELT LSST Main Author – Presentation Title Observatories in Chile: Where? ALMA CCAT* Nanten 2 ASTE Paranal Vista ACT 2 3 E-ELT* TAO* Apex CTA* Las Campanas GMT* Polar Bear Simons Obs. La Silla 1 Tololo SOAR Gemini LSST* 6 Giant Magellan Telescope (GMT): Will be the largest in the world in 2022 25 meters in diameter “Price”: US$1340 million First light: 2023 Enclosure is 62 m high Groundbreaking research in: . Exoplanets and their atmospheres . Dark matter . Distant objects . Unknown unknowns 7 Just how tall is the GMT? 46 meters 8 Giant Magellan Telescope (GMT): The world’s largest optical telescope Korea Sao Paulo, Brazil Texas A&M Arizona New partners are welcome! Main Author – Presentation Title 9 Central mirror casting – Sep 2015 Ohara glass, Japan Main Author – Presentation Title Casting of Mirror #5 – Nov 2017 Main Author – Presentation Title Las Campanas Observatory Meteorological towers Enclosure diameter Summit GMT – 56 m offices Telescope foundation – 22 m Main Author – Presentation Title Excavation of the telescope enclosure August 2018-January 2019 Main Author – Presentation Title 13 Main Author – Presentation Title 14 Main Author – Presentation Title 15 GMT Enclosure Altura: 60,5 m Main Author – Presentation Title GMT Facilities Safety first Residence with 92 rooms – maximum capacity: 228 . Large kitchen and dining room . Recreation area Wide road ready – allows access to wide loads Hard-rock excavation for telescope enclose and auxiliary buildings is ready Water and telescope/enclosure cooling system utilities IT . Datacenter: AWS . Chile backup (Las Campanas & Santiago) Main Author – Presentation Title Water & Utilities Package Construction Main Author – Presentation Title ¡Muchas gracias! Contact: Dr. Mauricio Pilleux – [email protected] 19.

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Overview and Status of the Giant Magellan Telescope Project
Invited Paper Overview and Status of the Giant Magellan Telescope Project Patrick J. McCarthy*,a,b, James Fansona, Rebecca Bernsteina,b, David Ashbyc, Bruce Bigelowa, Nune Boyadjiana, Antonin Boucheza, Eric Chauvina, Eduardo Donosoa, Jose Filgueiraa, Robert Goodricha, Frank Groarka, George Jacobya, Eric Pearcea aGMTO Corporation, 451 N. Halstead St., Suite 250, Pasadena, CA 91107, USA bCarnegie Observatories, 813 Santa Barbara St., Pasadena, CA 91101, USA cLarge Binocular Telescope Observatory, Tucson AZ ABSTRACT The Giant Magellan Telescope Project is in the construction phase. Production of the primary mirror segments is underway with four of the seven required 8.4m mirrors at various stages of completion and materials purchased for segments five and six. Development of the infrastructure at the GMT site at Las Campanas is nearing completion. Power, water and data connections sufficient to support the construction of the telescope and enclosure are in place and roads to the summit have been widened and graded to support transportation of large and heavy loads. Construction pads for the support buildings have been graded and the construction residence is being installed. A small number of issues need to be resolved before the final design of the telescope structure and enclosure can proceed and the GMT team is collecting the required inputs to the decision making process. Prototyping activities targeted at the active and adaptive optics systems are allowing us to finalize designs before large scale production of components begins. Our technically driven schedule calls for the telescope to be assembled on site in 2022 and to be ready to receive a subset of the primary and secondary mirror optics late in the year.
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Experimental Facilities in Latin America
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Precision Optics Manufacturing and Control for Next-Generation Large
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Effective Aperture 3.6–4.9 M) 4.7 M 186″ Segmented, MMT (6×1.8 M) F
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Manufacture of 8.4 M Off-Axis Segments: a 1/5 Scale Demonstration
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Support for Site Testing of the European Extremely Large Telescope: Precipitable Water Vapour Over La Silla†
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HATS-7B: a HOT SUPER NEPTUNE TRANSITING a QUIET K DWARF STAR* G
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